Low-temperature gas opacity: æsopus: a versatile and quick computational tool

Astronomy and Astrophysics

Volumn 508, Issue 3, 2009, Pages 1539-1569

  Marigo, P ^a   Aringer, B ^b,c  

^a UNIVERSITY OF PADOVA   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^c UNIVERSITY OF VIENNA   (Austria)

Author keywords

Atomic processes; Equation of state; Molecular processes; Stars: abundances; Stars: AGB and post AGB; Stars: atmospheres

Indexed keywords

ASYMPTOTIC GIANT BRANCH STARS; ATOMIC PROCESS; CHEMICAL COMPOSITIONS; CHEMICAL MIXTURES; COLLISION-INDUCED ABSORPTION; COMPUTATIONAL TIME; COMPUTATIONAL TOOLS; DEGREE OF FREEDOM; DISCRETE SOURCES; EQUATION OF STATE; EVOLUTIONARY MODELS; GLOBULAR CLUSTERS; IDEAL GAS; LOW TEMPERATURES; LOW-TEMPERATURE REGIME; MASSIVE STARS; METAL ABUNDANCES; MOLECULAR ABSORPTION; MOLECULAR PROCESSES - STARS; MOLECULAR SPECIES; NEW TOOLS; ROSSELAND MEAN OPACITY; SOLAR ABUNDANCES; STATE VARIABLES; UTILITY SOFTWARE; WOLF-RAYET; MOLECULAR PROCESS; STARS: ABUNDANCES; STARS: ATMOSPHERE;

ATOMS; EQUATIONS OF STATE OF GASES; GAS ABSORPTION; GAS MIXTURES; OPACITY; SODIUM; STARS; THERMAL LOGGING; MIXTURES; PHASE INTERFACES;

PHASE INTERFACES; GASES;

EID: 72849147717     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912598     Document Type: Article

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